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Bright spots on Ceres

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The bright material is only millions of years old; cryovolcanism may not have stopped completely as there is evidence of hydrated NaCl, and a thin haze, observed through variation in brightness, still present today, thought to be due to sublimating ice. Ice would not last long in such warm conditions
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of these spots was speculated to be due to some kind of outgassing, and subsequent closer images helped scientists determine that it is a material with a high level of reflection, and suggested ice and salt as possibilities. These bright features have an albedo of about 40%, four times brighter than
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suggested "a meteorite strike either shook covering material off the salty ice or heated it so that salty water rose to the surface as a geyser. The water escaped into space and now, only the salt remains." A haze that fills around half of Occator crater and that does not extend over its rim
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images led to widespread reports in the media about the bright spots, including in news sources, astronomy magazines, and science magazines. An informal NASA poll during May offered the following ideas for the nature of the spots: ice, volcanos, geysers, salt deposits, rock, or other.
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Further analysis of Dawn's low-altitude data indicates two sources: melting of crustal ices by impact, and a deeper brine reservoir (of sodium carbonate and/or ammonium chloride), near or in the mantle. Hanami planum is a topographic high but a
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Vu, Tuan H.; Hodyss, Robert; Johnson, Paul V.; Choukroun, Mathieu (July 2017). "Preferential formation of sodium salts from frozen sodium-ammonium-chloride-carbonate brines – Implications for Ceres' bright spots".
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Quick, Lynnae C.; Buczkowski, Debra L.; Ruesch, Ottaviano; Scully, Jennifer E.C.; Castillo-Rogez, Julie; Raymond, Carol A.; Schenk, Paul M.; Sizemore, Hannah G.; Sykes, Mark V. (1 March 2019).
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De Sanctis, M; Ammannito, E; Raponi, A; Frigeri, A; Ferrari, M; Carrozzo, F; Ciarniello, M; Formisano, M; Rousseau, B; Tosi, F.; Zambon, F.; Raymond, C. A.; Russell, C. T. (10 August 2020).
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Raymond, C; Ermakov, A; Castillo-Rogez, J; Marchi, S; Johnson, B; Hesse, M; Scully, J; Buczkowski, D (2020). "Impact-driven mobilization of deep crustal brines on dwarf planet Ceres".
56:. The largest and brightest component of the cluster is in the center of the crater, with dimmer spots located towards this crater's eastern rim. Early in the orbital phase of the 243:
Reflectivity studies from September 2015 suggest that the spots are probably salts rather than ice, implying that Ceres's interior is somehow delivering fresh salt to the surface.
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magazine, that at low angles a haze can be seen in but not outside of the crater, and speculated that this could be sublimated vapor from ice, possibly linked to the bright spots.
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periodically appears around Spot 5, the best known bright spot, adding credence to the idea that some sort of outgassing or volcanism is occurring.
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Park, R; Konopliv, A; Ermakov, A; Castillo-Rogez, J (2020). "Evidence of non-uniform crust of Ceres from Dawn's high-resolution gravity data".
1113:"A Possible Brine Reservoir Beneath Occator Crater: Thermal and Compositional Evolution and Formation of the Cerealia Dome and Vinalia Faculae" 1258: 825: 804: 1701: 2480: 457: 353: 1334: 508:
De Sanctis, M. C.; et al. (29 June 2016). "Bright carbonate deposits as evidence of aqueous alteration on (1) Ceres".
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that percolated to the surface in various locations causing the "bright spots", including those in Occator crater.
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Schenk, P; Scully, J; Buczkowski, D; Sizemore, H; Schmidt, B; Pieters, C; Neesemann, A; O'Brien, D (2020).
1112: 1056:"Impact heat driven volatile redistribution at Occator crater on Ceres as a comparative planetary process" 1694: 1921: 1269: 1784: 1316: 622: 166:
exposed to the vacuum of space, so that would suggest it is being brought to the surface to this day.
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The brightest cluster of spots ("Spot 5") is located in an 80-kilometer (50 mi) crater called
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On 9 December 2015, scientists reported that the bright spots on Ceres may be related to a type of
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The brightest cluster of spots ("Spot 5") is located in an 80-kilometer (50 mi) crater called
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Sky and Telescope magazine - Dawn Sees Ceres Bright Spots and More By Emily Poore July 30, 2015
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LPSC 2015: First results from Dawn at Ceres: provisional place names and possible plumes
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Now Appearing At a Dwarf Planet Near You: NASA's Dawn Mission to the Asteroid Belt
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McCartney, Gretchen; JHautaluoma, Grey; Johnson, Alana (10 August 2020).
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Video (3:34): Ceres "Bright Spots" - Mystery solved (10 August 2020)
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Cerealia and Vinalia Faculae stand out against the dark surface in
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Dawn at Ceres: A haze in Occator crater? Posted by Andrew Rivkin
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Scully, J; Schenk, P; Castillo-Rogez, J; Buczkowski, D (2020).
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Ceres' Mysterious Bright Spots Aren't Made of Ice After All
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Asteroid specialist A. Rivkin noted, in an article by
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Solar System bodies formerly considered to be planets
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O); the spots were also found to be associated with
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USGS Astrogeology Research Program. 722:. USGS Astrogeology Research Program. 651:"Cryovolcanism on Dwarf Planet Ceres" 481: 416:Landau, Elizabeth (9 December 2015). 327: 293: 836: 191:Spots on Ceres from different angles 738:Gazetteer of Planetary Nomenclature 720:Gazetteer of Planetary Nomenclature 649:Krummheuer, Birgit (6 March 2017). 13: 1104: 891:Witze, Alexandra (18 March 2015). 726: 708: 14: 2927: 1709: 1259:Ceres Photo Journal at NASA's JPL 1246: 921:"What's the spot on World Ceres?" 2890: 2889: 1466: 1460: 365:Feltman, Rachel (10 July 2015). 211:International Astronomical Union 65:the average of Ceres's surface. 16:Surface features discovered 2015 1200: 1143: 982: 971: 837:Amos, Jonathan (2 March 2015). 819: 803:Rivkin, Andrew (21 July 2015). 796: 744: 661: 642: 552: 501: 267:, the tallest mountain on Ceres 209:. These names were approved by 1722:List of possible dwarf planets 950:Cofield, Calla (22 May 2015). 863:Beatty, Kelly (3 March 2015). 475: 435: 1: 482:Lewin, Sarah (29 June 2016). 391:Rayman, Marc (8 April 2015). 276: 1129:10.1016/j.icarus.2018.07.016 7: 562:Planetary and Space Science 258: 137:) or ammonium bicarbonate ( 10: 2932: 1176:10.1038/s41467-020-15973-8 1080:10.1038/s41467-020-17184-7 296:"USGS: Ceres nomenclature" 173: 2916:Surface features of Ceres 2885: 2856: 2783: 2471: 2338: 2151: 2128: 2023: 1965: 1942: 1935: 1918: 1765: 1717: 1651: 1620: 1574: 1518: 1510:2006 definition of planet 1482: 1475: 1458: 1440: 1424: 1343: 1330: 1312: 1304: 1229:10.1038/s41550-020-1019-1 1030:10.1038/s41550-020-1168-2 694:10.1038/s41550-020-1138-8 574:10.1016/j.pss.2017.04.014 255:, likely by buried ices. 169: 72:, particularly a form of 807:. The Planetary Society 1253:Dawn mission home page 294:Staff (13 July 2015). 253:isostatic compensation 192: 31: 1726:Former dwarf planets 1156:Nature Communications 1060:Nature Communications 919:Staff (25 May 2015). 328:Staff (6 July 2015). 190: 174:Further information: 24: 1575:Possible trojans and 1541:Franz Xaver von Zach 1531:Carl Friedrich Gauss 1495:Definition of planet 218:Swinburne University 1221:2020NatAs...4..748P 1168:2020NatCo..11.3680S 1162:(1): article 3680. 1072:2020NatCo..11.3679S 1066:(1): article 3679. 1022:2020NatAs...4..741R 898:Scientific American 870:Sky & Telescope 686:2020NatAs...4..786D 530:10.1038/nature18290 522:2016Natur.536...54D 445:. 15 December 2015. 371:The Washington Post 237:Sky & Telescope 1636:Ceres Polar Lander 931:on 15 October 2015 758:on 15 October 2015 213:26 November 2016. 193: 93:ammonia-rich clays 60:mission, the high 32: 2903: 2902: 2881: 2880: 1677: 1676: 1616: 1615: 1561:Johann Elert Bode 1536:Francis Wollaston 1456: 1455: 778:"Chris Russel at" 734:"Vinalia Faculae" 716:"Cerealia Facula" 81:magnesium sulfate 2923: 2893: 2892: 2874: 2872: 2871: 2849: 2839: 2829: 2819: 2809: 2799: 2785:Detached objects 2776: 2774: 2773: 2764: 2762: 2761: 2752: 2750: 2749: 2740: 2738: 2737: 2728: 2726: 2725: 2716: 2714: 2713: 2704: 2702: 2701: 2692: 2682: 2680: 2679: 2670: 2660: 2650: 2640: 2630: 2623: 2621: 2620: 2611: 2601: 2591: 2589: 2588: 2579: 2569: 2567: 2566: 2557: 2547: 2537: 2527: 2517: 2507: 2497: 2464: 2454: 2444: 2434: 2424: 2414: 2412: 2411: 2402: 2392: 2382: 2372: 2362: 2352: 2331: 2329: 2328: 2319: 2309: 2299: 2289: 2279: 2269: 2259: 2249: 2239: 2229: 2219: 2209: 2207: 2206: 2197: 2187: 2144: 2121: 2119: 2118: 2109: 2099: 2089: 2079: 2069: 2059: 2049: 2016: 2006: 1996: 1940: 1939: 1930: 1924: 1704: 1697: 1690: 1681: 1680: 1642:Calathus Mission 1609: 1607: 1606: 1592: 1590: 1589: 1585:(185105) 2006 SV 1480: 1479: 1470: 1464: 1341: 1340: 1299: 1292: 1285: 1276: 1275: 1266: 1241: 1240: 1209:Nature Astronomy 1204: 1198: 1197: 1187: 1147: 1141: 1140: 1108: 1102: 1101: 1091: 1051: 1042: 1041: 1010:Nature Astronomy 1005: 996: 995:, 1 October 2015 986: 980: 975: 969: 968: 966: 964: 947: 941: 940: 938: 936: 927:. 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1728: 1727: 1725: 1723: 1720: 1719: 1716: 1712: 1711:Dwarf planets 1705: 1700: 1698: 1693: 1691: 1686: 1685: 1682: 1670: 1667: 1665: 1662: 1660: 1657: 1656: 1654: 1650: 1643: 1640: 1637: 1634: 1632: 1630: 1626: 1625: 1623: 1619: 1608: 1599: 1597: 1596:1372 Haremari 1594: 1591: 1582: 1581: 1579: 1573: 1567: 1564: 1562: 1559: 1557: 1554: 1552: 1549: 1547: 1544: 1542: 1539: 1537: 1534: 1532: 1529: 1527: 1524: 1523: 1521: 1517: 1511: 1508: 1506: 1503: 1501: 1498: 1496: 1493: 1491: 1488: 1487: 1485: 1481: 1478: 1474: 1469: 1463: 1449: 1446: 1445: 1443: 1439: 1433: 1430: 1429: 1427: 1423: 1417: 1414: 1412: 1409: 1407: 1404: 1402: 1399: 1397: 1394: 1392: 1389: 1387: 1384: 1382: 1379: 1377: 1374: 1372: 1369: 1367: 1364: 1362: 1359: 1357: 1354: 1352: 1349: 1348: 1346: 1342: 1339: 1336: 1329: 1323: 1320: 1318: 1315: 1314: 1311: 1307: 1300: 1295: 1293: 1288: 1286: 1281: 1280: 1277: 1271: 1267: 1262: 1260: 1257: 1254: 1251: 1250: 1238: 1234: 1230: 1226: 1222: 1218: 1214: 1210: 1203: 1195: 1191: 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Index


Occator crater
faculae
Ceres
Dawn spacecraft
Occator
albedo
salt
brine
hydrated
magnesium sulfate
ammonia-rich clays
sublimated
sodium carbonate
brine
Occator (crater)
Occator

Cerealia
Vinalia
International Astronomical Union
Swinburne University
Sky & Telescope
gravity low
isostatic compensation
Ahuna Mons
Sublimation


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